The connection between stellar activity cycles and magnetic field topology

Abstract

Zeeman Doppler imaging has successfully mapped the large-scale magnetic fields of stars over a large range of spectral types, rotation periods and ages. When observed over multiple epochs, some stars show polarity reversals in their global magnetic fields. On the Sun, polarity reversals are a feature of its activity cycle. In this paper, we examine the… (More)

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Cite this paper

@inproceedings{See2017TheCB, title={The connection between stellar activity cycles and magnetic field topology}, author={Vladimir See and Moira Jardine and A. A. Vidotto and Boro Saikia and J. Bouvier and Raafat P. Fares and Colin P. Folsom and Simon G. Gregory and Gaitee A. J. Hussain and J.-F. Donati and Sangeeta Saikia and Craig Folsom and S. V. Je↵ers and Siobhan Marsden and J. Morin and Claudine Moutou and Jos{\'e} Jailson Costa do Nascimento and Pierre Petit and I. A. Waite}, year={2017} }